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import numpy as np
import pywcs
import pyfits
from updatewcs import wcsutil
from numpy import sqrt, arctan2
def output_wcs(list_of_wcsobj, ref_wcs=None, outwcs=None):
fra_dec = np.vstack([w.footprint for w in list_of_wcsobj])
delta_fdec = (fra_dec[:,1].max()-fra_dec[:,1].min())
crval2 = fra_dec[:,1].min()+ delta_fdec/2.
delta_fra = (fra_dec[:,0].max()-fra_dec[:,0].min())
min_ind = fra_dec[:,0].argmin()
crval1 = (fra_dec[min_ind,0]+ (delta_fra/2.)*np.cos((fra_dec[min_ind,1]-crval2)*np.pi/180))
crval = np.array([crval1,crval2])
if outwcs is None:
if ref_wcs == None:
ref_wcs = list_of_wcsobj[0]
outwcs = undistortWCS(ref_wcs)
outwcs.wcs.crval = crval
outwcs.pscale = sqrt(outwcs.wcs.cd[0,0]**2 + outwcs.wcs.cd[1,0]**2)*3600.
outwcs.orientat = arctan2(outwcs.wcs.cd[0,1],outwcs.wcs.cd[1,1]) * 180./np.pi
else:
outwcs.pscale = sqrt(outwcs.wcs.cd[0,0]**2 + outwcs.wcs.cd[1,0]**2)*3600.
outwcs.orientat = arctan2(outwcs.wcs.cd[0,1],outwcs.wcs.cd[1,1]) * 180./np.pi
tanpix = outwcs.wcs.s2p(fra_dec)['pixcrd']
outwcs.naxis1 = int(np.ceil(tanpix[:,0].max() - tanpix[:,0].min()))
outwcs.naxis2 = int(np.ceil(tanpix[:,1].max() - tanpix[:,1].min()))
crpix = np.array([outwcs.naxis1/2., outwcs.naxis2/2.])
outwcs.wcs.crpix = crpix
tanpix = outwcs.wcs.s2p(fra_dec)['pixcrd']
newcrpix = np.array([crpix[0]+np.ceil(tanpix[:,0].min()), crpix[1]+np.ceil(tanpix[:,1].min())])
newcrval = outwcs.wcs.p2s([newcrpix])['world'][0]
outwcs.wcs.crval = newcrval
return outwcs
def undistortWCS(wcsobj):
assert isinstance(wcsobj, pywcs.WCS)
import coeff_converter
cx, cy = coeff_converter.sip2idc(wcsobj)
crpix1 = wcsobj.wcs.crpix[0]
crpix2 = wcsobj.wcs.crpix[1]
xy = np.array([(crpix1,crpix2),(crpix1+1.,crpix2),(crpix1,crpix2+1.)],dtype=np.double)
offsets = np.array([wcsobj.ltv1, wcsobj.ltv2])
px = xy + offsets
#order = wcsobj.sip.a_order
pscale = wcsobj.idcscale
#pixref = np.array([wcsobj.sip.SIPREF1, wcsobj.sip.SIPREF2])
tan_pix = apply_idc(px, cx, cy, wcsobj.wcs.crpix, pscale, order=1)
xc = tan_pix[:,0]
yc = tan_pix[:,1]
am = xc[1] - xc[0]
bm = xc[2] - xc[0]
cm = yc[1] - yc[0]
dm = yc[2] - yc[0]
cd_mat = np.array([[am,bm],[cm,dm]],dtype=np.double)
# Check the determinant for singularity
_det = (am * dm) - (bm * cm)
if ( _det == 0.0):
print 'Singular matrix in updateWCS, aborting ...'
return
#lin_wcsobj = wcsutil.HSTWCS(instrument=wcsobj.instrument)
lin_wcsobj = pywcs.WCS() #instrument=wcsobj.instrument)
cd_inv = np.linalg.inv(cd_mat)
lin_wcsobj.wcs.cd = np.dot(wcsobj.wcs.cd, cd_inv)
lin_wcsobj.orientat = arctan2(lin_wcsobj.wcs.cd[0,1],lin_wcsobj.wcs.cd[1,1]) * 180./np.pi
lin_wcsobj.pscale = sqrt(lin_wcsobj.wcs.cd[0,0]**2 + lin_wcsobj.wcs.cd[1,0]**2)*3600.
return lin_wcsobj
def apply_idc(pixpos, cx, cy, pixref, pscale= None, order=None):
#pixpos must be already corrected for ltv1/2
if cx == None:
return pixpos
if order is None:
print 'Unknown order of distortion model \n'
return pixpos
if pscale is None:
print 'Unknown model plate scale\n'
return pixpos
# Apply in the same way that 'drizzle' would...
_cx = cx/pscale
_cy = cy/ pscale
_p = pixpos
# Do NOT include any zero-point terms in CX,CY here
# as they should not be scaled by plate-scale like rest
# of coeffs... This makes the computations consistent
# with 'drizzle'. WJH 17-Feb-2004
_cx[0,0] = 0.
_cy[0,0] = 0.
dxy = _p - pixref
# Apply coefficients from distortion model here...
c = _p * 0.
for i in range(order+1):
for j in range(i+1):
c[:,0] = c[:,0] + _cx[i][j] * pow(dxy[:,0],j) * pow(dxy[:,1],(i-j))
c[:,1] = c[:,1] + _cy[i][j] * pow(dxy[:,0],j) * pow(dxy[:,1],(i-j))
return c
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